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Автор A D Erlykin
Автор A W Wolfendale
Дата выпуска 1995-08-01
dc.description An analysis is made of the contribution of unresolved 'sources', mainly active galactic nuclei (AGN), to the high energy diffuse gamma-ray flux using several approaches. It is shown that the AGN contribution is almost certainly the dominant source of this flux. The implications for the origin of ultra-high energy cosmic rays-which themselves generate gamma rays by interacting with the cosmic microwave background-are discussed.
Формат application.pdf
Издатель Institute of Physics Publishing
Название The high energy extragalactic gamma-ray background and its relevance to the origin of ultra-high energy cosmic rays
Тип paper
DOI 10.1088/0954-3899/21/8/011
Electronic ISSN 1361-6471
Print ISSN 0954-3899
Журнал Journal of Physics G: Nuclear and Particle Physics
Том 21
Первая страница 1149
Последняя страница 1165
Аффилиация A D Erlykin; Lebedev (P.N.) Phys. Inst., Moscow, Russia
Аффилиация A W Wolfendale; Lebedev (P.N.) Phys. Inst., Moscow, Russia
Выпуск 8

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